Table 6
Priors used for the analysis of KOI-188, KOI-195, KOI-192, and KOI-830.
| Parameter | KOI-188 | KOI-195 | KOI-192 | KOI-830 | |
|
|
|||||
| Ephemerides and orbital parameters | |||||
| Orbital period P [d] |  (3.79702, 5 × 10-5) |
(3.21752, 5 × 10-5) |
(10.29100, 5 × 10-5) |
(3.52563, 5 × 10-5) |
|
| Transit epoch T0 [BJDTDB - 2 454 900] |
|
|
|
|
|
| Orbital inclination i [°] |
|
|
|
|
|
| Orbital eccentricity e | 0 | 0 | β(0.867,3.03) | 0 | |
| Argument of periastron ω [°] | 90 | 90 |
|
90 | |
|
|
|||||
| Transit parameters | |||||
| Radius ratio rp/R⋆ |
|
|
|
|
|
| Linear limb-darkening coefficient ua |
|
|
|
|
|
| Quadratic limb-darkening coefficient ub |
|
|
|
|
|
|
|
|||||
| Radial velocity parameters | |||||
| Systemic velocity υ0 [km s-1] |
|
|
|
|
|
| Radial-velocity semi-amplitude K [km s-1] |
|
|
|
|
|
|
|
|||||
| Stellar parameters | |||||
| Effective temperature Teff [K] |
|
|
|
|
|
| Iron abundance [Fe/H] [dex] |
|
|
|
|
|
| Bulk density ρ⋆ [ρ⊙] |  (1.19, 0.22, 0.17) |
(1.13, 0.26) |
 (0.27, 0.09, |
(1.46, 0.31) |
|
| 0.66, 0.33, -0.56) | |||||
|
|
|||||
| System parameters | |||||
| Distance from Earth D [pc] |
|
|
|
|
|
| Interstellar extinction E(B − V) [mag] |
|
|
|
|
|
|
|
|||||
| Instrumental parameters | |||||
| Kepler season 0 LC: | |||||
| Jitter [%] |
|
|
|
|
|
| Contamination [%] |
|
|
|
|
|
| Out-of-transit flux |
|
|
|
|
|
| Kepler season 0 SC: | |||||
| Jitter [%] |
|
|
|
– | |
| Contamination [%] |
|
|
|
– | |
| Out-of-transit flux |
|
|
|
– | |
| Kepler season 1 LC: | |||||
| Jitter [%] |
|
|
|
|
|
| Contamination [%] |
|
|
|
|
|
| Out-of-transit flux |
|
|
|
|
|
| Kepler season 1 SC: | |||||
| Jitter [%] |
|
– |
|
– | |
| Contamination [%] |
|
– |
|
– | |
| Out-of-transit flux |
|
– |
|
– | |
| Kepler season 2 LC: | |||||
| Jitter [%] |
|
|
|
|
|
| Contamination [%] |
|
|
|
|
|
| Out-of-transit flux |
|
|
|
|
|
| Kepler season 2 SC: | |||||
| Jitter [%] |
|
|
|
– | |
| Contamination [%] |
|
|
|
– | |
| Out-of-transit flux |
|
|
|
– | |
| Kepler season 3 LC: | |||||
| Jitter [%] |
|
|
|
|
|
| Contamination [%] |
|
|
|
|
|
| Out-of-transit flux |
|
|
|
|
|
| Kepler season 3 SC: | |||||
| Jitter [%] |
|
|
|
– | |
| Contamination [%] |
|
|
|
– | |
| Out-of-transit flux |
|
|
|
– | |
| HARPS-N 2012: | |||||
| Jitter [m s-1] |
|
|
|
– | |
| Offset [m s-1] |
|
|
|
|
|
| HARPS-N 2013: | |||||
| Jitter [m s-1] |
|
|
|
|
|
| Offset [m s-1] | 0 | 0 | 0 | 0 | |
| SED: | |||||
| Jitter [mag] |
|
|
|
|
|
Notes. 
denotes a Uniform prior between a and b; 
denotes a Jeffreys distribution between a and b; 
denotes a Normal distribution with a mean of μ and a width of σ2; 
denotes an asymmetric Normal distribution with mean μ, upper width 
, and lower width 
; 
denotes a Normal distribution with a mean of μ, a width of σ2, and limited by a Uniform distribution between a and b; 
denotes a Bi-Normal distribution with means of μ1 and μ2, widths of 
and 
, and ΔA is the amplitude ratio between the two Normal distributions such that 
; 
denotes a Sine distribution between a and b; and finally β(a,b) denotes a Beta distribution with parameters a and b (Kipping 2013).
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